HEDM作为固体推进剂组分的评价(Ⅰ):几种环状硝胺的计算研究

对近几年新合成的几个环状硝胺化合物的能量性能进行了计算分析,并与HMX作了比较,提出了评价其作为推进剂组分潜力的方法.初步分析结果表明,BCSDX和HNIW具有高能量密度的特点,是比较有希望的高能量密度材料.     

高置信度验模方法及若干问题探讨

本文论述导弹系统仿真建模、验模及一体化研究问题，概述建模的主要内容，提出验模的一般观点，分析现有验模方法用于导弹系统仿真模型验证时的困难和局限性，并提出高置信度验模方法的基本特征和方法研究的技术途径。同时，就如何保证仿真模型验证结果具有高的置信水平所关联的问题进行探讨。     

基于显式表达式的空间目标最大碰撞概率分析

最大碰撞概率的计算在空间目标碰撞风险评估中具有重要意义。基于碰撞概率的显式 表达式,利用一元函数和二元函数求极值的方法分别讨论了目标误差椭球形状固定和不定两 种情况下最大碰撞概率的计算方法,得到了两种情况下最大碰撞概率的表达式。对于误差椭 球形状固定的情况得到了碰撞概率最大时两目标位置协方差的取值,对于误差椭球不定情况 得到了碰撞概率最大时径向联合方差的取值和水平面内联合方差所满足的关系。分析了最大 碰撞概率的影响因素,讨论了水平面内误差方差的耦合特性。对今年二月发生的美俄卫星碰 撞事件进行了分析,得到误差椭球任意形状时最大碰撞概率为1.864E-3。
     

Spectrophotometric diagnostics of energy characteristics and conductance of the auroral ionosphere from satellite: 1. Specific methods,accuracy problems,and instrumentation requirements

One of the most important tasks of space research is to find a way of real-time monitoring of the space environment conditions around the Earth. This is necessary in order to provide warning about the threats of critical failures in ground-based and space technological systems, thus providing for their stable and secure operation. In view of this concern, methods of diagnostics of ionospheric energy and electrodynamic characteristics continue to be developed on the basis of spectral and photometric measurements, analyzing the glow intensity of emissions of the upper atmosphere observed from above. Serial panoramic monochromatic maps of the intensity of luminosity of the upper atmosphere emissions measured from orbiting detectors can serve as a main data source for such an analysis. In this paper we consider the principal aspects of the method, and, on this basis, the instrumentation requirements are formulated.     

基于i.MX21的视频采集编码系统设计与实现

介绍基于i.MX21处理器的视频采集编码系统的设计,该系统从CSI接口获取CMOS传感器采集的图像数据,使用eMMA多媒体加速器实现数据的MPEG4格式压缩,重点介绍CSI驱动程序和视频数据采集编码的实现.     

Dynamics of a gyrostat satellite with the vector of gyrostatic moment in the principal plane of inertia

Dynamics of a gyrostat satellite moving along a circular orbit in a central Newtonian field of force is investigated. In a particular case, when the gyrostatic moment vector lies in one of the satellite’s principal central planes of inertia, all positions of equilibrium are determined, and the conditions of their existence are analyzed. Also determined are bifurcation values of dimensionless parameters, at which the number of equilibrium positions changes. As a result of analysis of the generalized energy integral, for each equilibrium orientation the sufficient conditions of stability are derived. Evolution of the regions where the sufficient conditions of stability are valid is investigated under variation of the system’s dimensionless parameters.     

Intermittency of solar wind density fluctuations and its relation to sharp density changes

The paper presents the study of turbulent properties of the solar wind plasma, namely, the intermittency of fluctuations of the solar wind ion flux in the earlier unexplored region of comparatively high frequencies (0.01–1 Hz). Special attention is given to a comparison of intermittency for solar wind observation intervals containing sharp (shorter than 10 min) and high-amplitude (greater than 20%) changes of the ion flux to intervals without such changes. The solar wind observation intervals containing sharp changes of the flux are found to be essentially more intermittent than the intervals of quiet solar wind. Such a comparison allows one to reveal the fundamental difference in turbulent properties of the solar wind depending on the presence or absence of sharp boundaries in plasma structures.     

Spaceflight results in increase of thick filament but not thin filament proteins in the paramyosin mutant of Caenorhabditis elegans

We have investigated the effect of microgravity during spaceflight on body-wall muscle fiber size and muscle proteins in the paramyosin mutant of Caenorhabditis elegans. Both mutant and wild-type strains were subjected to 10 days of microgravity during spaceflight and compared to ground control groups. No significant change in muscle fiber size or quantity of the protein was observed in wild-type worms; where as atrophy of body-wall muscle and an increase in thick filament proteins were observed in the paramyosin mutant unc-15(e73) animals after spaceflight. We conclude that the mutant with abnormal muscle responded to microgravity by increasing the total amount of muscle protein in order to compensate for the loss of muscle function.     

变结构方法在导弹控制中的应用

本文针对模型参数大范围变化的反舰导弹控制问题，将变结构控制方法作了成功的应用。通过在滑动模态曲面附近引入切换区，使抖动现象削弱；在控制受限情况下，改变滑动误差反馈增益，使系统具有很快的收敛速度。该方法应用于某型反舰导弹控制，仿真结果证明系统能够适应大范围参数变，并具有良好的动态性能和强鲁棒性。     

Launch cost reduction by the reuse of the core stage of Ariane 5

The high cost of launching payloads into Earth orbit is a main limiting factor on the development of space. In order to reduce the high cost of launch, reuse of (parts of) the launch vehicle is needed. This study analyses the possibilities of recovering and reusing the core stage of Ariane 5. Recovery of the core stage sets demands on re-entry trajectory, attitude, stability, thermal protection, structural strength, terminal deceleration, salt water protection, recovery and refurbishment. All these subject areas require solutions to their individual problems. Added subsystems to the stage are defined and their mass is determined. These masses are used to determine the financial feasibility of the recovery concept, by weighing the payload demise and operational cost against the gains of reduced production cost. It is concluded that the recovery is technologically feasible, using a detachable ablative heat shield on the nose of the stage and a stabilisation device (an inflatable drag cone), a parachute system and an engine enclosure device. Total mass of these systems is 1320 kg, with financial savings amounting to $8.5 million per flight.